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JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18

Authors: Fengwu Sun, Jakob M. Helton, Eiichi Egami, Kevin N. Hainline, George H. Rieke, Christopher N. A. Willmer, Daniel J. Eisenstein, Benjamin D. Johnson, Marcia J. Rieke, Brant Robertson, Sandro Tacchella, Stacey Alberts, William M. Baker, Rachana Bhatawdekar, Kristan Boyett, Andrew J. Bunker, Stephane Charlot, Zuyi Chen, Jacopo Chevallard, Emma Curtis-Lake, A. Lola Danhaive, Christa DeCoursey, Zhiyuan Ji, Jianwei Lyu, Roberto Maiolino, Wiphu Rujopakarn, Lester Sandles, Irene Shivaei, Hannah Übler, Chris Willott, Joris Witstok

Fengwu Sun et al 2024 The Astrophysical Journal 961 .

Provider: AAS Journals

Caption: Figure 5.

1D profile of HDF850.1 along the direction of major axis in the image plane. Surface brightness profile in the rest-frame V band (F356W) is shown in gray, and stellar mass profile (Section 3.5) is shown in red. Half-light and half-mass radii are highlighted as vertical dashed lines. The half-mass–radius is consistent with the half-light radius of 1 mm dust continuum measured by Neri et al. (2014). Empirical PSF profile in the F444W band is shown in solid black line for comparison. All profiles are normalized to 1 at the centroids.

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